“…The STILT‐produced backward trajectories are used to calculate footprints—the sensitivity of concentrations at the receptor due to upwind surface influences at each 0.01° grid box (ppm (μmol m −2 s −1 ) −1 ). More specifically, surface flux footprints f ( x r , t r | x i , y j , t m ) for a given receptor located at x r at time t r from an upwind source at ( x i , y j ) and past time t m are a function of the number of Lagrangian particles residing in the planetary boundary layer (PBL) for that upwind location as given by the equation below: where m air is the molecular weight of air, h is the height of the volume in which the surface fluxes are diluted over, ρ is the average density of all particles, N tot is the total number of particles, and Δ t p , i , j , k is the amount of time a particle p spends within the volume at location ( x i , y j ) and time t m (Lin et al, ; Mallia et al, ).…”